Bose-Einstein condensation may occur in a constant magnetic field
arXiv:hep-th/9510191 · doi:10.1016/0370-2693(96)00430-3
Abstract
Bose-Einstein condensation of charged scalar and vector particles may actually occur in presence of a constant homogeneous magnetic field, but there is no critical temperature at which condensation starts. The condensate is described by the statistical distribution. The Meissner effect is possible in the scalar, but not in the vector field case, which exhibits a ferromagnetic behavior.
Latex, 9 pages
References in corpus (3)
Cited by in corpus (22)
- Quantum Magnetic Collapse
- Magnetized strange quark matter and magnetized strange quark stars
- Cold ideal equation of state for strongly magnetized neutron-star matter: effects on muon production and pion condensationn
- Antikaon condensation in neutron stars
- Anisotropic Pressures in Very Dense Magnetized Matter
- Phase structure of the QCD vacuum in a magnetic field at low temperature
- Chiral thermodynamics in a magnetic field
- Magnetic catalysis of a charged Bose-Einstein condensate
- Bose-Einstein condensation in dense nuclear matter and strong magnetic fields
- On Bose-Einstein Condensation in any Dimension
- Pair Production of charged vector bosons in supercritical magnetic fields at finite temperatures
- Thermodynamical properties of a neutral vector boson gas in a constant magnetic field
- Diamagnetism versus Paramagnetism in charged spin-1 Bose gases
- Thermodynamics of rotating Bose gases in a trap
- Simple criterion for the occurrence of Bose-Einstein condensation and the Meissner-Ochsenfeld effect
- Two-step condensation of the charged Bose gas
- Phase diagram for charged scalars in a magnetic field at finite temperature
- Bose-Einstein condensation of the magnetized ideal Bose gas
- A non-relativistic magnetized vector boson gas at any temperature
- Magnetized vector boson gas at any temperature
- One-loop omega-potential of charged massive particles in a constant homogeneous magnetic field at high temperatures
- Anomalous enhancement of Neel order in the square lattice Heisenberg model under fictitious magnetic field